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25 February 1993 X-ray adaptive mirror: principle and state of the art
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Abstract
Adaptive optics systems have proven their efficiency for obtaining high resolution images in the field of large astronomical telescopes. The same techniques can be applied to correct x-ray mirror shapes. The paper describes the principle of an adaptive x-ray mirror system (mirror architecture, measurement subassembly, control unit). In the second part, first results obtained during the design study of the ESRF adaptive x-ray mirror are given. The possibility of achieving cylindrical or elliptical mirror surfaces using adaptive optics techniques are suggested.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jean-Paul Gaffard, R. Ravelet, and Corinne Boyer "X-ray adaptive mirror: principle and state of the art", Proc. SPIE 1739, High Heat Flux Engineering, (25 February 1993); https://doi.org/10.1117/12.140513
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